SDO HMI 2014-11-05 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.32 | 0.00 | 10.19 | -21.63 | 76.92 | -2.86 | 176.11 | 0.4479 | 659.8 | 460.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.71 | -20.20 | 84.40 | 4.63 | 190.49 | 0.4177 | 873.0 | 711.5 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -15.67 | 83.92 | 4.14 | 191.70 | 0.3444 | 815.0 | 629.1 | |
| 0.00 | 1.99 | 0.00 | 1.08 | -19.51 | 83.81 | 4.04 | 189.47 | 0.4053 | 772.0 | 527.4 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -21.63 | 82.13 | 2.36 | 185.07 | 0.4353 | 658.0 | 548.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.93 | 81.91 | 2.14 | 184.17 | 0.4708 | 683.0 | 414.3 | |
| 0.00 | 1.73 | 0.00 | 0.94 | -20.87 | 80.63 | 0.85 | 181.90 | 0.4218 | 896.0 | 646.0 | |
| 0.00 | 1.99 | 0.00 | 1.08 | -20.67 | 79.67 | -0.10 | 179.78 | 0.4185 | 705.0 | 623.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -22.18 | 78.26 | -1.52 | 176.82 | 0.4431 | 762.0 | 587.0 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -20.38 | 77.36 | -2.41 | 174.52 | 0.4156 | 819.0 | 703.5 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -20.64 | 76.88 | -2.90 | 173.52 | 0.4206 | 777.0 | 676.6 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -20.57 | 76.50 | -3.28 | 172.65 | 0.4203 | 728.0 | 606.9 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -20.74 | 75.41 | -4.36 | 170.33 | 0.4255 | 818.0 | 664.6 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -24.29 | 71.61 | -8.16 | 164.69 | 0.4920 | 498.0 | 421.0 | |
| 0.00 | 2.07 | 0.00 | 1.31 | -28.08 | 58.07 | -21.70 | 148.19 | 0.6213 | -567.0 | -501.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |